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Fig. 4

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Number counts of galaxies per 0.5 mag per arcmin2 in the U band for the fields in our survey, which have been derived by single-mode photometry. We see that there is very good agreement between our estimates and previous studies (Capak et al. 2004; Eliche-Moral et al. 2006; Rovilos et al. 2009; Grazian et al. 2009).

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